The radio source population at high frequency: follow-up of the 15-GHz 9C survey

被引:37
作者
Bolton, RC
Cotter, G
Pooley, GG
Riley, JM
Waldram, EM
Chandler, CJ
Mason, BS
Pearson, TJ
Readhead, ACS
机构
[1] Univ Cambridge, Cavendish Lab, Dept Phys, Cavendish Astrophys, Cambridge CB3 0HE, England
[2] Oxford Astrophys, Oxford OX1 3RH, England
[3] Natl Radio Astron Observ, VLA, Array Operat Ctr, Socorro, NM 87801 USA
[4] NRAO, Greenbank Telescope, Green Bank, WV 24944 USA
[5] CALTECH, Pasadena, CA 91125 USA
关键词
surveys; galaxies : active; radio continuum : general;
D O I
10.1111/j.1365-2966.2004.08207.x
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We have carried out extensive radio and optical follow-up of 176 sources from the 15-GHz 9th Cambridge survey. Optical identifications have been found for 155 of the radio sources; optical images are given with radio maps overlaid. The continuum radio spectrum of each source spanning the frequency range 1.4-43 GHz is also given. Two flux-limited samples are defined, one containing 124 sources complete to 25 mJy and one of 70 sources complete to 60 mJy. Between one-fifth and one-quarter of sources from these flux-limited samples display convex radio spectra, rising between 1.4 and 4.8 GHz. These rising-spectrum sources make up a much larger fraction of the radio source population at this high selection frequency than in lower frequency surveys. We find that by using non-simultaneous survey flux density measurements at 1.4 and 15 GHz to remove steep-spectrum objects, the efficiency of selecting objects with spectra rising between 1.4 and 4.8 GHz (as seen in simultaneous measurements) can be raised to 49 per cent without compromising the completeness of the rising-spectrum sample.
引用
收藏
页码:485 / 521
页数:37
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